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Observations of the V=0 S(2) Line of Molecular Hydrogen at 12.28μm in the Orion Molecular Cloud
Published online by Cambridge University Press: 14 August 2015
Abstract
The 12.28μm pure rotational line of molecular hydrogen has been detected in emission from the region of vibration-rotation line emission in Orion. The line shapes, widths, and velocities are similar to those observed in the V=1 → 0 transition at 2.12μm. Constraints imposed by these new results on models of the emitting region are discussed.
- Type
- Research Article
- Information
- Symposium - International Astronomical Union , Volume 87: Interstellar Molecules , 1980 , pp. 465 - 468
- Copyright
- Copyright © Reidel 1980